the theoretical limit, while Si is cheap. New systems must perform! Metal oxides Cu2 O (6%) Bi2 FeCrO6 (8%) Co3 O4 (<1%) Metal sulfides SnS (5%) Cu2 ZnSn(S,Se)4 (14%) Sb2 S3 (8%) Metal halides CsSnI3 (10%) CH3 NH3 PbI3 (22%) CH(NH2 )2 PbI3 (20%) Examples of materials studied for thin-film photovoltaics
what can we learn? B. Kesterites (A2 BCX4 ) – danger, low voltage! C. Tin Sulfides (Ax Bx ) – two elements, many problems. D. Beyond (Ax By Xz ) – exploring new materials.
absorption (Eg ~ 1.6 eV) • Light electron and hole masses (conductive) • Easy to synthesise (cheap and scalable) Advanced Features • Large dielectric constants: carrier separation (weak excitons) and transport (low scattering) • Slow e-h recombination: low losses, large VOC o Relativistic effects – spin-orbit coupling o Polar domains – dynamic fluctuations
Holes Effective semiconductors Lattice Vibrations Symmetry breaking and carrier separation Molecular Rotations Large static dielectric constant Ions and Charged Defects “Self healing” and hysteresis What is moving in perovskite solar cells? Acc. Chem. Res. 49, 528 (2016)
Holes Effective semiconductors Lattice Vibrations Symmetry breaking and carrier separation Molecular Rotations Large static dielectric constant Ions and Charged Defects “Self healing” and hysteresis What is moving in perovskite solar cells? Acc. Chem. Res. 49, 528 (2016)
what can we learn? B. Kesterites (A2 BCX4 ) – danger, low voltage! C. Tin Sulfides (Ax Bx ) – two elements, many problems. D. Beyond (ABX) – exploring new materials.
Cu2 ZnSn(S,Se)4 (CZTS) solar cell 1988; 12.6% by IBM (2014); 13.8% report from DGIST (2016) High-thoughput Density Functional Theory: Phys. Rev. B 79, 165211 (2009)
+ ZnS • Cation disorder, e.g. Cu-Zn; Cu-Sn; Zn-Sn mixing • Deep level defects, i.e. fast non-radiative recombination • Interface reactions, e.g. MoS2 formation at back contact Challenging for experiment, theory and simulation! Issues for Kesterite Solar Cells Wallace, Mitzi and Walsh, ACS Energy Letters 2, 776 (2017) Champion solar cells suffer from large voltage deficits, e.g. for CZTS (Eg = 1.5 eV), VOC = 0.7 V
what can we learn? B. Kesterites (A2 BCX4 ) – danger, low voltage! C. Tin Sulfides (Ax Bx ) – two elements, many problems. D. Beyond (ABX) – exploring new materials.
L. A. Burton and A. Walsh, J. Phys. Chem. C 116, 24262 (2012) Sn(II) 5s25p0 Sn(IV) 5s05p0 Sterically active lone pair [asymmetric coordination] e.g. SnO, SnS Octahedral or tetrahedral environments e.g. SnO2 , SnS2
thin-films using a variety of deposition techniques Golan, Nano Lett 15, 2174 (2015); Skelton et al, APL Materials 5, 036101 (2017) • Previously misidentified as “zincblende” phase • Structure solved on basis of X-ray and electron diffraction • Phonon stable (PBEsol) • Eg = 1.7 eV (HSE06 + SOC) • Chiral: non-linear optics
what can we learn? B. Kesterites (A2 BCX4 ) – danger, low voltage! C. Tin Sulfides (Ax Bx ) – two elements, many problems. D. Beyond (ABX) – exploring new materials.
Direct optical bandgap (1 – 2 eV) • Easy to deposit and scale-up production • Semiconductor with low carrier concentrations • Tolerant to impurities and microstructure • Chemically stable at interfaces • Workfunction matched to electrical contacts
108, 112103 (2016) Trivalent cation with monovalent & divalent anions V VI VII Bi O F Sb S Cl Se Br Te I Ferroelectrics Photocatalysts Solar Cell Absorbers Topological Conductors
108, 112103 (2016) Trivalent cation with monovalent & divalent anions V VI VII Bi O F Sb S Cl Se Br Te I Ferroelectrics Photocatalysts Solar Cell Absorbers Topological Conductors
energy conversion. Challenge is translation to efficient devices. Theory and simulation can help to identify and overcome bottlenecks. Project Collaborators: Keith Butler, Jarvist Frost, Jonathan Skelton, Lucy Whalley, Ruoxi Yang, Suzy Wallace (ICL); Simon Billinge (Columbia); Mark van Schilfgaarde (Kings); Bruno Erhler (AMOLF) Funding: ERC; EPSRC; Royal Society; Leverhulme Slides: https://speakerdeck.com/aronwalsh